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Thermodynamics, stability and Hawking–Page transition of Kerr black holes from Rényi statistics [PDF]
European Physical Journal C: Particles and Fields, 2017 Thermodynamics of rotating black holes described by the Rényi formula as equilibrium and zeroth law compatible entropy function is investigated. We show that similarly to the standard Boltzmann approach, isolated Kerr black holes are stable with respect ...
Viktor G. Czinner, Hideo Iguchi
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Entropy bound of horizons for charged and rotating black holes
Physics Letters B, 2015 We revisit the entropy product, entropy sum and other thermodynamic relations of charged and rotating black holes. Based on these relations, we derive the entropy (area) bound for both event horizon and Cauchy horizon.
Wei Xu, Jia Wang, Xin-he Meng
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Jackiw-Teitelboim gravity and rotating black holes
Journal of High Energy Physics, 2019 We show that the free energy at low temperatures for near-extremal black holes is correctly obtained from the Jackiw-Teitelboim (JT) model of gravity. Our arguments apply to all black holes, including rotating ones, whose metric has a near-horizon AdS2 ...
Upamanyu Moitra +3 more
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Journal of High Energy Physics, 2012 We investigate the critical behaviour of charged and rotating AdS black holes in d spacetime dimensions, including effects from non-linear electrodynamics via the Born-Infeld action, in an extended phase space in which the cosmological constant is ...
David Kubiznák, Robert B Mann
exaly +3 more sources
A note on the entropy of rotating BPS AdS7 × S4 black holes
Journal of High Energy Physics, 2018 In this note we show that the entropy of BPS, rotating, electrically charged AdS7 × S 4 black holes can be obtained by an extremization principle involving a particular combination of anomaly coefficients of the six-dimensional N=20 $$ \mathcal{N}=\left ...
Seyed Morteza Hosseini +2 more
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Thin accretion disks around rotating black holes in 4D Einstein–Gauss–Bonnet gravity
European Physical Journal C: Particles and Fields, 2021 Recently, Kumar and Ghosh have derived Kerr-like rotating black hole solutions in the framework of four-dimensional Einstein–Gauss–Bonnet theory of gravity and investigated the black hole shadow. Using the steady-state Novikov–Thorne model, we study thin
Mohaddese Heydari-Fard +2 more
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Kretschmann Scalar for a Kerr-Newman Black Hole [PDF]
, 1999 I have derived the Kretschmann scalar for a general black hole of mass m, angular momentum per unit mass a, and electric charge Q. The Kretschmann scalar gives the amount of curvature of spacetime, as a function of position near (and within) a black hole.
Henry, Richard C.
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Journal of High Energy Physics, 2023 We consider black holes generically sourced by quantum matter described by regular wavefunctions. This allows for integrable effective energy densities and the removal of Cauchy horizons in spherically symmetric configurations.
Roberto Casadio +2 more
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Chern-Simons dilaton black holes in 2+1 dimensions [PDF]
, 2016 We construct rotating magnetic solutions to the three-dimensional Einstein-Maxwell-Chern-Simons-dilaton theory with a Liouville potential. These include a class of black hole solutions which generalize the warped AdS black holes.
Clément, Gérard +2 more
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Applications of Thermodynamic Geometries to Conformal Regular Black Holes: A Comparative Study
Universe, 2023 In this paper, we investigate the thermal stability and thermodynamic geometries of non-rotating/rotating charged black holes. For these black holes, we apply barrow entropy to determine the physical quantities such as mass and temperature of the system ...
Abdul Jawad +2 more
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